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Calibration of a Terrestrial Laser Scanner - Institute of Geodesy and ...

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138 3. <strong>Calibration</strong> <strong>of</strong> <strong>Terrestrial</strong> <strong>Laser</strong> <strong>Scanner</strong>the derived horizontal distances to the computed spheres <strong>and</strong> the nominal horizontal distances providedby the interferometer for the 'free' adjustment <strong>and</strong> for the 'fix' adjustment<strong>and</strong> for both diameters <strong>of</strong> 12 cm<strong>and</strong> 15 cm. The point cloud, from which the spheres were calculated, were acquired by the scanning mode'superhigh'. The figure shows that the results obtained by 'fix' adjustmentare much better than these ob¬tained by 'free' adjustment. It can be assumed that the results <strong>of</strong> the 'free' adjustment can be improved byapplying an additive constant because all distances are 3 mm to 4 mm to short8. The deviations increase sig¬nificantly for the 'free' adjustment from 10 m <strong>and</strong> thus agree with the results <strong>of</strong> the diameters comparison.The results based on the scanning modes 'high' <strong>and</strong> 'middle' confirm the findings. Consideringadjustment, the range from which the deviations grow strongly decreases from 10 m upthe 'free'to several meters.100000800001Ifpoints on sphere• 12cmhyperbola1 • 15cmhyperbola(AC'o 60000Q.M—oI 400003C2000011\\\\\\\ XN»\^^r__"0 2 4 6 8 10 12 14 16 18 20range [m]Figure 3.17: Development <strong>of</strong> the number <strong>of</strong>points defining a sphere acquired by scanning at different ranges. Sphereswith diameters <strong>of</strong> 12 cm <strong>and</strong> 15 cm were scanned by the scanning mode 'superhigh'. The curves define a hyperbola.The spheres to be modeled are based on a point cloud which vary in the quantity <strong>of</strong> points. The quantity<strong>of</strong> the laser points decreases with the range <strong>and</strong> with the scanning modes from 'superhigh' to 'preview'. InFigure 3.17 the number <strong>of</strong> points belonging to the sphereswith 12 cm <strong>and</strong> 15 cm are shown <strong>and</strong> include thecorresponding adjustment hyperbolae for the scanning mode 'superhigh'. The adjustment hyperbolae arebased on the mathematical formula [Bronstein <strong>and</strong> Semendjajew, 1999]:f(x)=a-xb. (3.5)It can be seen that the number <strong>of</strong> points decreases rapidly according to the anglezontal <strong>and</strong> the vertical encoder. The parameters <strong>of</strong> the adjustment hyperbolaTherefore, the power b <strong>of</strong> both hyperbolae fit each other, which means the gradients<strong>and</strong> the hyperbola decreases similarly.increment <strong>of</strong> the hori¬are summarized in Table 3.2.<strong>of</strong> the lines are identicalThe scale factor a states for the number <strong>of</strong> points accordingto therange <strong>of</strong> 1 m, which have to be different for the spheres because <strong>of</strong> the different diameters. Considering theother scanning modes, 'high' <strong>and</strong> 'middle', the number <strong>of</strong> points is lowered by a factor <strong>of</strong> four <strong>and</strong> sixteen,respectively. This reduction in the number <strong>of</strong> points is based on a sub-sampling, which means only eachnth pixel in the horizontal <strong>and</strong> vertical directions is stored depending on the highest angle resolution. Forthe scanning mode 'high', the sub-sampling is n 2 <strong>and</strong> for the scanning modes 'middle' <strong>and</strong> 'preview',=the sub-sampling is n 4 <strong>and</strong> = n 16, respectively. Thus, the number <strong>of</strong> points hitting = a spheremaximum distance for scanning a spherecan be estimated.<strong>and</strong> the8Since the spheres to be scanned are not only aligned in the x-direction or in the y-direction with respect to the local scanner systemthe resulting Cartesian coordinates <strong>of</strong> the spheres based on the azimuth <strong>and</strong> the horizontal distance corrected by the additive constanthas to be calculated. This procedure can be applied also on slope distances in 3D-space.

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